Zobrazeno 1 - 10
of 43 833
pro vyhledávání: '"Barclay As"'
Following the universal availability of generative AI systems with the release of ChatGPT, automatic detection of deceptive text created by Large Language Models has focused on domains such as academic plagiarism and "fake news". However, generative
Externí odkaz:
http://arxiv.org/abs/2412.15253
Autor:
Crossfield, Ian J. M., Polanski, Alex S., Robertson, Paul, Murphy, Joseph Akana, Turtelboom, Emma V., Luque, Rafael, Beatty, Thomas, Daylan, Tansu, Isaacson, Howard, Brande, Jonathan, Kreidberg, Laura, Batalha, Natalie M., Huber, Daniel, Rhem, Maleah, Dressing, Courtney, Kane, Stephen R., Bossett, Malik, Gagnebin, Anna, Kroft, Maxwell A., Premnath, Pranav H., Rogers, Claire J., Collins, Karen A., Latham, David W., Watkins, Cristilyn N., Ciardi, David R., Howell, Steve B., Savel, Arjun B., Berlind, Perry, Calkins, Michael L., Esquerdo, Gilbert A., Mink, Jessica, Clark, Catherine A., Lund, Michael B., Matson, Rachel A., Everett, Mark E., Schlieder, Joshua E., Matthews, Elisabeth C., Giacalone, Steven, Barclay, Thomas, Zambelli, Roberto, Plavchan, Peter, Ellingson, Taylor, Bowen, Michael, Srdoc, Gregor, McLeod, Kim K., Schwarz, Richard P., Barkaoui, Khalid, Kamler, Jacob, Murgas, Felipe, Palle, Enric, Narita, Norio, Fukui, Akihiko, Relles, Howard M., Bieryla, Allyson, Girardin, Eric, Massey, Bob, Stockdale, Chris, Lewin, Pablo, Papini, Riccardo, Guerra, Pere, Conti, Dennis M., Yalcinkaya, Selcuk, Basturk, Ozgur, Mourad, Ghachoui
Sub-Neptunes - volatile-rich exoplanets smaller than Neptune - are intrinsically the most common type of planet known. However, the formation and nature of these objects, as well as the distinctions between sub-classes (if any), remain unclear. Two p
Externí odkaz:
http://arxiv.org/abs/2411.16836
Autor:
Flågan, Sigurd, Itoi, Joe, Shandilya, Prasoon K., Kavatamane, Vinaya K., Mitchell, Matthew, Lake, David P., Barclay, Paul E.
Photoinduced modification of second-harmonic generation mediated by nitrogen vacancy (NV) centres in a diamond cavity is observed. Excitation of NV centres quenches the device's second-harmonic emission, and is attributed to modification of $\chi^{(2
Externí odkaz:
http://arxiv.org/abs/2412.06792
Autor:
Shandilya, Prasoon K., Kavatamane, Vinaya K., Flågan, Sigurd, Lake, David P., Sukachev, Denis, Barclay, Paul E.
The photodynamics of diamond nitrogen-vacancy (NV) centers limits their performance in many quantum technologies. Quenching of photoluminescence, which degrades NV readout, is commonly ascribed to a dark state that is not fully understood. Using a na
Externí odkaz:
http://arxiv.org/abs/2411.10638
Autor:
Johnson, Ted M, Kelahan, Cameron, Mandell, Avi M., Dhahbi, Ashraf, Hammond, Tobi, Barclay, Thomas, Kostov, Veselin B., Villanueva, Geronimo L.
We present the Variable Star PhasE Curve (VSPEC) Collection, a set of Python packages for simulating combined-light spectroscopic observations of 3-dimensional exoplanet atmospheres in the presence of stellar variability and inhomogeneity. VSPEC uses
Externí odkaz:
http://arxiv.org/abs/2410.21190
Image classification usually requires connectivity and access to the cloud which is often limited in many parts of the world, including hard to reach rural areas. TinyML aims to solve this problem by hosting AI assistants on constrained devices, elim
Externí odkaz:
http://arxiv.org/abs/2408.08215
Autor:
Ghachoui, M., Rackham, B. V., Dévora-Pajares, M., Chouqar, J., Timmermans, M., Kaltenegger, L., Sebastian, D., Pozuelos, F. J., Eastman, J. D., Burgasser, A. J., Murgas, F., Stassun, K. G., Gillon, M., Benkhaldoun, Z., Palle, E., Delrez, L., Jenkins, J. M., Barkaoui, K., Narita, N., de Leon, J. P., Mori, M., Shporer, A., Rowden, P., Kostov, V., Fűrész, G., Collins, K. A., Schwarz, R. P., Charbonneau, D., Guerrero, N. M., Ricker, G., Jehin, E., Fukui, A., Kawai, Y., Hayashi, Y., Esparza-Borges, E., Parviainen, H., Clark, C. A., Ciardi, D. R., Polanski, A. S., Schleider, J., Gilbert, E. A., Crossfield, I. J. M., Barclay, T., Dressing, C. D., Karpoor, P. R., Softich, E., Gerasimov, R., Davoudi, F.
Publikováno v:
A&A 690, A263 (2024)
We present the validation of two TESS super-Earth candidates transiting the mid-M dwarfs TOI-6002 and TOI-5713 every 10.90 and 10.44 days, respectively. The first star (TOI-6002) is located $32.038\pm0.019$ pc away, with a radius of $0.2409^{+0.0066}
Externí odkaz:
http://arxiv.org/abs/2408.00709
Autor:
Solanki, Siddhant, Cieplak, Agnieszka M., Schnittman, Jeremy, Baker, John G., Barclay, Thomas, Barry, Richard K., Kostov, Veselin, Kruse, Ethan, Olmschenk, Greg, Powell, Brian P., Silva, Stela Ishitani, Torres, Guillermo
We identify $240$ short-period ($P \lesssim 10$ days) binary systems in the TESS data, $180$ of which are heartbeat binaries (HB). The sample is mostly a mix of A and B-type stars and primarily includes eclipsing systems, where over $30\%$ of the sou
Externí odkaz:
http://arxiv.org/abs/2407.14421
Autor:
Schaeper, Otto Cranwell, Spencer, Lesley, Scognamiglio, Dominic, El-Sayed, Waleed, Whitefield, Benjamin, Horder, Jake, Coste, Nathan, Barclay, Paul, Toth, Milos, Zalogina, Anastasiia, Aharonovich, Igor
The integration of van der Waals (vdW) materials into photonic devices has laid out a foundation for many new quantum and optoelectronic applications. Despite tremendous progress in the nanofabrication of photonic building blocks from vdW crystals, t
Externí odkaz:
http://arxiv.org/abs/2407.13475
Autor:
Sikora, James T., Rowe, Jason F., Splinter, Jared, Barat, Saugata, Dang, Lisa, Cowan, Nicolas B., Barclay, Thomas, Colón, Knicole D., Désert, Jean-Michel, Kane, Stephen R., Llama, Joe, Shivkumar, Hinna, Stassun, Keivan G., Quintana, Elisa V.
High-eccentricity gas giant planets serve as unique laboratories for studying the thermal and chemical properties of H/He-dominated atmospheres. One of the most extreme cases is HD 80606b -- a hot Jupiter orbiting a sun-like star with an eccentricity
Externí odkaz:
http://arxiv.org/abs/2407.12456